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Atoms and Stars IST 2420 and IST 1990

Atoms and Stars IST 2420 and IST 1990. Class 1 Winter 2006 Instructor: David Bowen Course web site: www.is.wayne.edu/drbowen/aasw06. Handouts. Class 1 Notes IST 2420 Syllabus Lab 1 Handout Midterm Questions For IST 1990 only: Syllabus Moodle. Tonight’s Schedule. Logistics IST 2420

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Atoms and Stars IST 2420 and IST 1990

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  1. Atoms and StarsIST 2420 and IST 1990 Class 1 Winter 2006 Instructor: David Bowen Course web site: www.is.wayne.edu/drbowen/aasw06 Atoms and Stars, Class 1

  2. Handouts • Class 1 Notes • IST 2420 Syllabus • Lab 1 Handout • Midterm Questions • For IST 1990 only: • Syllabus • Moodle Atoms and Stars, Class 1

  3. Tonight’s Schedule • Logistics • IST 2420 • Syllabus • Characteristics of science • Lab 1 • IST 1990 (2420 free to leave) • Moodle Atoms and Stars, Class 1

  4. Logistics • Food & beverage machines • Student Center is fairly close • Bathrooms • Water • Take care of your own trash! • We are guests here, and individual conduct should not get us kicked out. • For labs, repack equipment where you found it. Atoms and Stars, Class 1

  5. IST 2420 • Meets WSU Gen Ed requirement for • Physical Science (PS) • Natural Sciences (PS and LS) laboratory requirement • Initial the signin sheet • Check 1990 column for correct number of credits • If you are not on the list, add your name at the bottom – this is NOT registration!!! • Review of names Atoms and Stars, Class 1

  6. IST 2420 (main course) • Physical science content • Nature of atmosphere • Speed of light • Solar system • Early chemistry, atomic theory • Nature of physical science • History and context • Scientific method • Experimentation • Nature of scientific knowledge Atoms and Stars, Class 1

  7. IST 2420 • Review of syllabus • Contact information • Proof that I don’t mind being contacted • Textbooks and bookstore (Reader and Lab Manual are changed from all previous versions) • Topics • Grading scale (W, X, I) • Weights • Assignment schedule Atoms and Stars, Class 1

  8. Syllabus, continued • Lab reports: two parts turned in as one • Absence and Making up Work: labs, classes, exams • Exam Questions and Essay Topics • Essays • Example of Mathematics Used In This Course • Turning in assignments Atoms and Stars, Class 1

  9. Syllabus, continued • Grade Appeals • Educational Accessibility • Assessment by the 4th Week • Class Conduct • Late/Missing Assignments • Dropping Classes • Grading for Course withdrawals • Plagiarism Atoms and Stars, Class 1

  10. Assignments for next week • Buy Reader / Lab Manual • In Lab Manual, read General laboratory Instructions, Additional Laboratory Instructions and Experiments 1 and 2 • Report on Temperamental Can due • In Reader, through Page 25 Atoms and Stars, Class 1

  11. How Do We Know What Science Is? • Who says what the scientific method is? • We listen to what scientists say they do, and watch them doing it • For example, Huxley (1863) and Copi (1986). • Exception: Frances Bacon present “at the birth” ~ 1600 • Science is an open community, but to be taken seriously, you must take its methods and concerns seriously • Galileo, Newton, Einstein and others were “mainstream” at first, revolutionary later • No exact definition of science that everyone agrees to, so looking at examples is a good method Atoms and Stars, Class 1

  12. Definitions for Reading • In “We Are All Scientists,” Huxley uses “induction” and “deduction” without defining them • Induction: reasoning from a series of identical cases to a general conclusion • In the reading: green apples example • Deduction: reasoning from different pieces of evidence to a conclusion in a specific case • In the reading, missing teapot and spoons example Atoms and Stars, Class 1

  13. Overview Scientific Method (as opposed to content): • We will do more here than typical science course • Here, Atoms and Stars is about origins of modern Physical Science (“science”) 1500 - 1700 AD in Europe • Development of Greek philosophy in the area of science, and how it was overthrown by science Atoms and Stars, Class 1

  14. Overview (cont’d) • Scientific Method (cont’d): • Modern Physical Science has roots going back to prehistory • It still represents something new • Also part of the course – what happened: • Before the Greeks? • Between the Greeks and the development of science? • After the development? Atoms and Stars, Class 1

  15. Overview • During development of science, much transmission by and (circa 1700) interaction with religion. Religion will come up. Atoms and Stars, Class 1

  16. Overview • My views (so you can evaluate what I say): • Scientist, advocate of science - secure and reliable information to support action • At any time, science has limits, so it cannot be a complete basis for living: current shortcomings are human nature & interactions, place in world, purpose • Science skeptics be careful: science limits always expanding • Member of church (Quakers, or Society of Friends), have taught Sunday School, been clerk, secretary, given counsel within the church. • A liberal church - I am liberal within that church. • Also a Ph.D. physicist (technical qualification) Atoms and Stars, Class 1

  17. Overview • I make no claim to expertise in religion • You have right here to your beliefs, to state those beliefs, to question, to reject science • Grading on your understanding of the course material, including the basis for trusting science • Science makes truth claims - what is the basis for believing those claims? • I believe science and religion are compatible • Not all religious beliefs compatible with all science. • Once you reject some science, hard to stop • Science is interconnected Atoms and Stars, Class 1

  18. Overview • Two pillars of science: • Data / observations / experiments • These make science reliable • Hypotheses / laws / theories • These make science valuable Atoms and Stars, Class 1

  19. Overview • #1: Data / observations / experiments • Direct, not secondhand • Must be repeatable by anyone who cares to try • Often suggested by a hypotheses / law / theory, but must be repeatable even if you disagree • Anything important is repeated • Some things (speed of light) repeated for 100+ years • Improved technique triggers another round of measurements Atoms and Stars, Class 1

  20. Overview • #1: Data / observations / experiments (cont’d) • If data from different scientists disagree, discrepancy must be checked and resolved – not taken seriously until then • Results cannot depend on beliefs or preferences – such effects must be checked and resolved • Often data suggested by a theory, but data stand even if theory fails Atoms and Stars, Class 1

  21. Overview • #1: Data / observations / experiments (cont’d) • Must be recorded, not restricted or secret, with procedure (what you did, including preparation) and results (what you saw / measured) • So that others can repeat and verify your results • Journals and raw notes kept, will be reviewed if questions arise Atoms and Stars, Class 1

  22. Overview • #2. Hypotheses / laws / theories • Hypothesis: first step - a guess, explain the data • Law is older term, theory is newer term (less assured) • Accepted theory must: • Be capable of being disproven (falsifiability) • Explain all (vast majority) data • Discrepancies must be addressed and eventually resolved Atoms and Stars, Class 1

  23. Overview • #2. Hypotheses / laws / theories (cont’d) • Accepted theory must (continued): • Have direct evidence - not accepted just because rival theory fails • If two theories agree with data, must look for and do critical experiments that decide between them • If two theories are inconsistent, this must be eventually be fixed • Be productive - predict new, unsuspected measurements, new phenomena, new results, which must be tested and which must agree • Simpler theory preferred to more complicated Atoms and Stars, Class 1

  24. Overview • Typical sequence of advance (focus comes first and is assumed here): • Observation / Measurement • Description • Understanding (theory) • Often this is first association (statistical) then causal • Control or technology (especially last 50 years) • Science is progressive • Start in small area, expand Atoms and Stars, Class 1

  25. Overview • Science is progressive (cont’d) • Later theory / experiment can change earlier theory • Example: Einstein's 1915 General Theory of Relativity changed ideas about his 1905 Theory of Special Relativity • However, old results still correct but range extended • Scientific knowledge provisional – subject to change Atoms and Stars, Class 1

  26. Overview • Science is progressive (cont’d) • Scientific knowledge can change rapidly at the frontier • Later experiments can show errors in the first ones • Extending theory beyond data can introduce errors • Science is not: • Fair – theories do not have a right to be considered – someone must want to do this Atoms and Stars, Class 1

  27. Overview • Science is not: • Democratic – no votes, nor formal consensus, theories can come “back to life” (string theory) • Not based on authority – Newton and Einstein can be (were) wrong • Most scientists follow these rules but (with many scientists) there are many exceptions • Science works socially – check each other Atoms and Stars, Class 1

  28. Overview • Most scientists follow these rules but (with many scientists) there are many exceptions (continued) • Scientific arguments can be fierce • Issue about women and aggressive argument • Our heroes – the people who overthrew the established order • Instant success: prove someone else wrong • Scientists often become advocates of a theory • Social interaction corrects this Atoms and Stars, Class 1

  29. Overview • Scientists are skeptical about truth claims • Many strongly-held beliefs have been shown to be wrong, e.g. common ideas about space • Many purely rational arguments have been shown to be wrong – e.g. Aristotle Atoms and Stars, Class 1

  30. Lab • Form five Lab groups. Will generally be the same each lab session • If changes, max group size is six • Temperamental Can – handout • Each person keeps his/her data sheet • Report will be individual, with an answer for each Assignment 1 – 12. • Start heating water for Assignment 2 as soon as possible. This will take time to boil. Atoms and Stars, Class 1

  31. Lab • Discuss Assignment 1 before doing Assignment 2, and write individual answers. • Then do rest of Assignments, come back to Assignment 2, 3 and 4 at the end. IST 1990 continues after Atoms and Stars, Class 1

  32. Lab • Reports should include (but it is one report): • Raw Data Sheet: • Setting: your name, experiment number, title and date, full names of lab partners • Procedure: what you did • Observations: what you saw happen and measurements during the lab period. • Hypotheses where requested, identified as hypotheses and separated from the rest • Typed analysis: Calculations and answers to questions in the lab manual • Do not retype Data Sheet – it would be less reliable Atoms and Stars, Class 1

  33. Questions or comments?Lab session nowAfterwards, IST 1990 only Atoms and Stars, Class 1

  34. IST 1990 Atoms and Stars, Class 1

  35. Course Topic • Science and religion - the interaction • Free to hold your own religious beliefs, but course is about the range of ideas. Optional: where do yours fit in? • Range of beliefs is very wide • Religion is superior • No conflict, some conflict • Science is superior Atoms and Stars, Class 1

  36. IST 1990 • Review of syllabus • Course description • Working on your own • Textbooks (at Barnes & Noble Campus Bookstore. 313-577-2436) • Gould: science and religion are, and should be, separate – they deal with separate areas • Barbour: what is the range of attitudes? Matrix • (four credits only) Ruse: How to reconcile Catholic doctrines with science • www.bkstore.com/wayne • My notes will be on the course web site Atoms and Stars, Class 1

  37. IST 1990 • Review of syllabus • Assigned readings on course web site • Assignments and schedule • Participation in online discussion • Set up account this week • Essays (two or three depending on credits) • Standards for essays and participation Atoms and Stars, Class 1

  38. Moodle • Handout • techtools.culma.wayne.edu/moodle • Creating an account • Enrolment key: 1990w06 (it is zero, not oh) • Using Moodle • This course listed as "W06 IST 1990 Science and Religion" or "W06_1990" Atoms and Stars, Class 1

  39. Atoms and Stars, Class 1

  40. Moodle • What is there: • Participants (list of class) • Online users (class members online now) • Chat • Edit Profile • Forums • Assignments – turn in files – file names • Recent activity (everyone, since the last time) • Under Administration, Activity report (yours) • Link back to course web site • More coming (grades) Atoms and Stars, Class 1

  41. Moodle: keeping track • Moodle will keep excellent track of what you have done • Assignments (essays) • Postings (online discussion) Atoms and Stars, Class 1

  42. Moodle • Assigned postings (count towards course requirement for number of postings): • Introduce yourself • Starting out • Pictures • Warning about online courses • One week – two weeks is stretching it • Moodle warning – watch for message • Watch course web site and email (weekly) Atoms and Stars, Class 1

  43. Moodle • Do not expect instantaneous responses from me • You do not need to respond to everything – gets out of hand if you do • I usually do not respond to messages that I agree with • I always respond to messages that I disagree with • Responses as well as original messages count • In a public setting, be sure to log out Atoms and Stars, Class 1

  44. Questions or comments? Atoms and Stars, Class 1

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